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Your search keyword '"Simon de Kockere"' showing total 4 results
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4 results on '"Simon de Kockere"'

3. High-Energy and Ultra-High-Energy Neutrinos: A Snowmass White Paper

Author

Markus Ackermann, Mauricio Bustamante, Lu Lu, Nepomuk Otte, Mary Hall Reno, Stephanie Wissel, Sanjib K. Agarwalla, Jaime Alvarez-Muñiz, Rafael Alves Batista, Carlos A. Argüelles, Brian A. Clark, Austin Cummings, Sudipta Das, Valentin Decoene, Peter B. Denton, Damien Dornic, Zhan-Arys Dzhilkibaev, Yasaman Farzan, Alfonso Garcia, Maria Vittoria Garzelli, Christian Glaser, Aart Heijboer, Jörg R. Hörandel, Giulia Illuminati, Yu Seon Jeong, John L. Kelley, Kevin J. Kelly, Ali Kheirandish, Spencer R. Klein, John F. Krizmanic, Michael J. Larson, Kohta Murase, Ashish Narang, Remy L. Prechelt, Steven Prohira, Elisa Resconi, Marcos Santander, Victor B. Valera, Justin Vandenbroucke, Olga Vasil'evna Suvorova, Lawrence Wiencke, Shigeru Yoshida, Tianlu Yuan, Enrique Zas, Pavel Zhelnin, Bei Zhou, Luis A. Anchordoqui, Yosuke Ashida, Mahdi Bagheri, Aswathi Balagopal, Vedant Basu, James Beatty, Keith Bechtol, Nicole Bell, Abigail Bishop, Julia Book, Anthony Brown, Alexander Burgman, Michael Campana, Nhan Chau, Thomas Y. Chen, Alan Coleman, Amy Connolly, Janet M. Conrad, Pablo Correa, Cyril Creque-Sarbinowski, Zachary Curtis-Ginsberg, Paramita Dasgupta, Simon De Kockere, Krijn de Vries, Cosmin Deaconu, Abhishek Desai, Tyce DeYoung, Armando di Matteo, Dominik Elsaesser, Phillip Fürst, Kwok Lung Fan, Anatoli Fedynitch, Derek Fox, Erik Ganster, Martin Ha Minh, Christian Haack, Steffen Hallman, Francis Halzen, Andreas Haungs, Aya Ishihara, Eleanor Judd, Timo Karg, Albrecht Karle, Teppei Katori, Alina Kochocki, Claudio Kopper, Marek Kowalski, Ilya Kravchenko, Naoko Kurahashi, Mathieu Lamoureux, Hermes León Vargas, Massimiliano Lincetto, Qinrui Liu, Jim Madsen, Yuya Makino, Joseph Mammo, Zsuzsa Marka, Eric Mayotte, Kevin Meagher, Maximilian Meier, Lino Miramonti, Marjon Moulai, Katharine Mulrey, Marco Muzio, Richard Naab, Anna Nelles, William Nichols, Alisa Nozdrina, Erin O'Sullivan, Vivian OD́ell, Jesse Osborne, Vishvas Pandey, Ek Narayan Paudel, Alex Pizzuto, Mattias Plum, Carlos Pobes Aranda, Lilly Pyras, Christoph Raab, Zoe Rechav, Juan Rojo, Oscar Romero Matamala, Pierpaolo Savina, Frank Schroeder, Lisa Schumacher, Sergio Sciutto, Stephen Sclafani, Mohammad Ful Hossain Seikh, Manuel Silva, Rajeev Singh, Daniel Smith, Samuel Timothy Spencer, Robert Wayne Springer, Juliana Stachurska, Olga Suvorova, Ignacio Taboada, Simona Toscano, Matias Tueros, Jean Pierre Twagirayezu, Nick van Eijndhoven, Péter Veres, Abigail Vieregg, Winnie Wang, Nathan Whitehorn, Walter Winter, Emre Yildizci, Shiqi Yu, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Faculty of Sciences and Bioengineering Sciences, Elementary Particle Physics, and Physics

Subjects
Astrophysics and Astronomy, neutrino: energy: high, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Baikal, WIMP: dark matter, neutrino: flux, IceCube, neutrino: decay, neutrino: energy, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], neutrino: supernova, numerical calculations, KM3NeT, Particle Physics - Phenomenology, astro-ph.HE, new physics, hep-ex, ANITA, Astronomy and Astrophysics, hep-ph, neutrino: UHE, neutrino: propagation, neutrino: detector, Space and Planetary Science, [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph], [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Particle Physics - Experiment
Abstract

Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy physics. With energies far beyond solar, supernovae, atmospheric, and accelerator neutrinos, high-energy and ultra-high-energy neutrinos probe fundamental physics from the TeV scale to the EeV scale and beyond. They are sensitive to physics both within and beyond the Standard Model through their production mechanisms and in their propagation over cosmological distances. They carry unique information about their extreme non-thermal sources by giving insight into regions that are opaque to electromagnetic radiation. This white paper describes the opportunities astrophysical neutrino observations offer for astrophysics and high-energy physics, today and in coming years. Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy physics. With energies far beyond solar, supernovae, atmospheric, and accelerator neutrinos, high-energy and ultra-high-energy neutrinos probe fundamental physics from the TeV scale to the EeV scale and beyond. They are sensitive to physics both within and beyond the Standard Model through their production mechanisms and in their propagation over cosmological distances. They carry unique information about their extreme non-thermal sources by giving insight into regions that are opaque to electromagnetic radiation. This white paper describes the opportunities astrophysical neutrino observations offer for astrophysics and high-energy physics, today and in coming years.

Published
2022

4. Simulation of in-ice cosmic ray air shower induced particle cascades

Author

Simon De Kockere, Nick Van Eijndhoven, Krijn De Vries, Uzair Latif, Physics, Faculty of Sciences and Bioengineering Sciences, Elementary Particle Physics, General Botany and Nature Management, Amphibian Evolution Lab, Ecology and Systematics, Cell Genetics, and Biology

Subjects
astro-ph.HE, High Energy Astrophysical Phenomena (astro-ph.HE), Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astrophysics - High Energy Astrophysical Phenomena, Physics::Atmospheric and Oceanic Physics
Abstract

We present detailed microscopic simulations of high-energy cosmic-ray air showers penetrating high-altitude ice layers that can be found at the polar regions. We use a combination of the CORSIKA Monte Carlo code and the Geant4 simulation toolkit, and focus on the particle cascade that develops in the ice to describe its most prominent features. We discuss the impact of the ice layer on the total number of particles in function of depth of the air shower, and we give a general parameterization of the charge distribution in the cascade front in function of Xmax of the cosmic ray air shower, which can be used for analytical and semi-analytical calculations of the expected Askaryan radio emission of the in-ice particle cascade. We show that the core of the cosmic ray air shower dominates during the propagation in ice, therefore creating an in-ice particle cascade strongly resembling a neutrino-induced particle cascade. Finally, we present the results of microscopic simulations of the Askaryan radio emission of the in-ice particle cascade, showing that the emission is dominated by the shower core, and discuss the feasibility of detecting the plasma created by the particle cascade in the ice using RADAR echo techniques., Comment: 14 pages, 18 figures

Published
2022
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